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The Solar System I

Horizontales
On the opposite side of the Earth from the Sun
A ring of icy bodies outside of Neptune’s orbit
The exchange of incoming and outgoing radiation that warms a planet
Channels that appear to have been made by water or glaciers
Is seen when a rotating object moves with different periods of rotation
Verticales
Because they were first observed by Galileo in 1610
The space between the second and third rings of Saturn
Somewhat flattened at its poles
The direct change from a solid to a gas
Because of the rust in the iron-filled Martian soil.